Molecular absorption in Cen A on VLBI scales

H. J. van Langevelde; Y. Pihlstroem; A. Beasley

doi:10.1007/s10509-005-3699-5

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arXiv · astro-ph/0409147

Molecular absorption in Cen A on VLBI scales

H. J. van Langevelde·Y. Pihlstroem·A. Beasley

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Abstract

Centaurus A, the nearest AGN shows molecular absorption in the millimeter and radio regime. By observing the absorption with VLBI, we try to constrain the distribution of the gas, in particular whether it resides in the circumnuclear region. Analysis of VLBA observations in four OH and two H2CO transitions is presented here, as well as molecular excitation models parameterized with distance from the AGN. We conclude that the gas is most likely associated with the tilted molecular ring structure observed before in molecular emission and IR continuum. The formaldehyde absorption shows small scale absorption which requires a different distribution than the hydroxyl.

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H. J. van Langevelde, Y. Pihlstroem, A. Beasley. 2004-09-07. Molecular absorption in Cen A on VLBI scales. https://doi.org/10.1007/s10509-005-3699-5

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